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Observation of a Helioseismically Active Solar Flare with a Low Hard X-ray Flux up to 50 keV.
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- Astronomy Letters, 2024, v. 50, n. 3, p. 203, doi. 10.1134/S1063773724700026
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Statistics of Thermal Plasma Parameters and Non-Thermal X-Ray Spectra of Solar Flares with Helioseismic Response.
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- Astronomy Reports, 2023, v. 67, n. 11, p. 1216, doi. 10.1134/S1063772923110094
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- Article
Vortex Motions in the Solar Atmosphere: Definitions, Theory, Observations, and Modelling.
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- Space Science Reviews, 2023, v. 219, n. 1, p. 1, doi. 10.1007/s11214-022-00946-8
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- Article
Solar oblateness & asphericities temporal variations: Outstanding some unsolved issues.
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- Proceedings of the International Astronomical Union, 2021, v. 15, n. S354, p. 232, doi. 10.1017/S1743921319009918
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Realistic 3D MHD modeling of self-organized magnetic structuring of the solar corona.
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- Proceedings of the International Astronomical Union, 2021, v. 15, n. S354, p. 346, doi. 10.1017/S1743921320001532
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- Article
Resolving Power of Asteroseismic Inversion of the Kepler Legacy Sample.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S354, p. 107, doi. 10.1017/S1743921320001416
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- Article
Solar oblateness & asphericities temporal variations: Outstanding some unsolved issues.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S354, p. 232, doi. 10.1017/S1743921319009918
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- Publication type:
- Article
Realistic 3D MHD modeling of self-organized magnetic structuring of the solar corona.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S354, p. 346, doi. 10.1017/S1743921320001532
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- Article
Magnetic field generation in PMS stars with and without radiative core.
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- Proceedings of the International Astronomical Union, 2016, v. 12, n. S328, p. 30, doi. 10.1017/S1743921317003970
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Are tachoclines important for solar and stellar dynamos? What can we learn from global simulations.
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- Proceedings of the International Astronomical Union, 2016, v. 12, n. S328, p. 61, doi. 10.1017/S1743921317003982
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- Article
Exploring shallow sunspot formation by using Implicit Large-eddy simulations.
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- Proceedings of the International Astronomical Union, 2016, v. 12, n. S328, p. 117, doi. 10.1017/S1743921317003921
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- Article
Initiation and chromospheric effects of a M1.0 class solar flare from high-resolution multi-wavelength observations.
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- Proceedings of the International Astronomical Union, 2016, v. 12, n. S327, p. 103, doi. 10.1017/S1743921317003994
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Preface.
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- Proceedings of the International Astronomical Union, 2016, v. 12, n. S327, p. vii
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Spectroscopic UV observations of M1.0 class solar flare from IRIS satellite.
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- Proceedings of the International Astronomical Union, 2015, v. 11, n. S320, p. 64, doi. 10.1017/S174392131600034X
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- Article
Sunquakes and starquakes.
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- Proceedings of the International Astronomical Union, 2013, v. 9, n. S301, p. 349, doi. 10.1017/S1743921313014579
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- Article
NUMERICAL SIMULATIONS OF IMPULSIVELY EXCITED ACOUSTIC-GRAVITY WAVES IN A STELLAR ATMOSPHERE.
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- Acta Physica Polonica B, 2011, v. 42, n. 6, p. 1333, doi. 10.5506/APhysPolB.42.1333
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Realistic MHD simulations of magnetic self-organization in solar plasma.
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- Proceedings of the International Astronomical Union, 2010, v. 6, n. S274, p. 120, doi. 10.1017/S1743921311006703
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Investigations of solar plasma in the interior and corona from Solar Dynamics Observatory.
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- Proceedings of the International Astronomical Union, 2010, v. 6, n. S274, p. 287, doi. 10.1017/S1743921311007149
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Realistic MHD numerical simulations of solar convection and oscillations in inclined magnetic field regions.
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- Proceedings of the International Astronomical Union, 2009, v. 5, n. H15, p. 348, doi. 10.1017/S1743921310009713
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- Article
The future of helioseismology.
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- Proceedings of the International Astronomical Union, 2009, v. 5, n. H15, p. 352, doi. 10.1017/S1743921310009749
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Prediction of solar activity cycles by assimilating sunspot data into a dynamo model.
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- Proceedings of the International Astronomical Union, 2009, v. 5, n. S264, p. 202, doi. 10.1017/S1743921309992638
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- Article
Photospheric and Subphotospheric Dynamics of Emerging Magnetic Flux.
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- Space Science Reviews, 2008, v. 144, n. 1-4, p. 175, doi. 10.1007/s11214-009-9487-8
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Magnetic fields and dynamics of the Sun's interior.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S259, p. 147, doi. 10.1017/S1743921309030397
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Prediction of solar magnetic cycles by a data assimilation method.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S259, p. 235, doi. 10.1017/S1743921309030531
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Joint Discussion 8 Solar and stellar activity cycles.
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- Proceedings of the International Astronomical Union, 2006, v. 2, n. 14, p. 271, doi. 10.1017/S174392130701054X
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Properties of Flares-Generated Seismic Waves on the Sun.
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- Solar Physics, 2006, v. 238, n. 1, p. 1, doi. 10.1007/s11207-006-0190-6
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- Article
Helioseismic inferences on subsurface solar convection.
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- Proceedings of the International Astronomical Union, 2006, v. 2, n. S239, p. 113, doi. 10.1017/S1743921307000257
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Active Region Dynamics.
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- Space Science Reviews, 2006, v. 124, n. 1-4, p. 1, doi. 10.1007/s11214-006-9112-z
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Comparison of subsurface sound-speed structures of three active regions.
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- Proceedings of the International Astronomical Union, 2006, v. 2, n. S233, p. 75, doi. 10.1017/S1743921306001499
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- Article
Subphotospheric Structure of Sunspots and Active Regions.
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- Proceedings of the International Astronomical Union, 2004, v. 2004, n. IAUS223, p. 171, doi. 10.1017/S174392130400554X
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Dynamics and Structure of Supergranulation.
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- Solar Physics, 2004, v. 221, n. 1, p. 23, doi. 10.1023/B:SOLA.0000033363.15641.8f
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Structure Properties of Supergranulation and Granulation.
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- Solar Physics, 2004, v. 221, n. 1, p. 33, doi. 10.1023/B:SOLA.0000033368.00217.de
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- Article